Detector | Exposure (Original/High-E Flare Cleaned/Low-E Cleaned) | Image binning | Plate scale ("/pixel) | Bgd. level (orig/High-E flare cleaned/cleaned, counts/sq. arcmin/s) | GTI file | Bgd. light curves | Roll angle | CCD counts | Extra info |
---|---|---|---|---|---|---|---|---|---|
pn | 741 | 318 | 173 | 1.00 | 4.35 | 0.33/0.098/0.058 | Yes | orig clean | ccd1:15849 ccd2:14897 ccd3:9932 ccd4:16702 ccd5:12970 ccd6:9716 ccd7:12622 ccd8:11742 ccd9:7902 ccd10:13082 ccd11:10708 ccd12:7588 |
filter=Thin1 date-obs=2000-05-15T17:21:08 object=Canopus z+3.5 timedel=0.07 roll_angle=301.345306396 |
0 source(s) in memory Iteration: 2 Images: |pn |
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Python version = 2.5.4 (r254:67916, Aug 14 2009, 18:07:15) [GCC 4.1.1 20070105 (Red Hat 4.1.1-52)]
Headas version = 6.11
XAssist version = 1.000
SAS version = xmmsas_20110223_1801-11.0.0
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Tue Dec 27 22:08:08 2011
This data set was last accessed on Tue Dec 27 22:08:08 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0122901801
Position of field target = 6 44 45.78 -54 20 7.4
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = OK
Detection method = eboxdetect
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Log files: processing messages |error messages |all messages (very detailed) |source logs